28 October 2015Achromatic interfero-coronagraph with variable rotational shear: reducing of star leakage effect, white light nulling with lab prototype
Pavel Frolov,1 Inna Shashkova,1,2 Yuliya Bezymyannikova,3,4 Alexander Kiselev,1 Alexander Tavrov1
1Space Research Institute (Russia) 2Moscow Power Engineering Institute (Russia) 3Space Research Institute (Russian Federation) 4Moscow Institute of Physics and Technology (Russian Federation)
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Stellar coronagraphs with a small inner working angle have limited possibilities to detect exoplanets due to the star leakage effect caused by incomplete suppression of the star of finite angular size. We consider an improved instrument for direct imaging of exoplanets: common-path achromatic interfero-coronagraph with variable rotational shear (CP-ARC). CP-ARC reduces the star leakage effect by several orders of magnitude (with small angles of rotational shear relative to a fixed angle of 180 deg) with telescope size more than 1 m. Operation capacity of CP-ARC was experimentally verified by laser light nulling and white light nulling with lab prototype treated.
Pavel Frolov,Inna Shashkova,Yuliya Bezymyannikova,Alexander Kiselev, andAlexander Tavrov
"Achromatic interfero-coronagraph with variable rotational shear: reducing of star leakage effect, white light nulling with lab prototype," Journal of Astronomical Telescopes, Instruments, and Systems 2(1), 011002 (28 October 2015). https://doi.org/10.1117/1.JATIS.2.1.011002
Published: 28 October 2015
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Pavel Frolov, Inna Shashkova, Yuliya Bezymyannikova, Alexander Kiselev, Alexander Tavrov, "Achromatic interfero-coronagraph with variable rotational shear: reducing of star leakage effect, white light nulling with lab prototype," J. Astron. Telesc. Instrum. Syst. 2(1) 011002 (28 October 2015) https://doi.org/10.1117/1.JATIS.2.1.011002